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The Role of the CMB in Redshift Related Departures from the Gao–Solomon Relation

  • Authors: R. Tunnard, and T. R. Greve

2017 The Astrophysical Journal 849 37.

  • Provider: AAS Journals

Caption: Figure 6.

Demonstration that the loss of contrast against a hot CMB is not much alleviated for single lines of sight by using the HCN(2−1) line. For the parameters discussed in Section 2.2 the HCN(2−1) line is affected almost identically to the HCN(1−0) line. Results shown here for the hot and cold limits of 102 K and ﹩{10}^{0.5}﹩ K on the earlier models for ﹩{\bar{n}}_{{{\rm{H}}}_{2}}=1\times {10}^{4}﹩ cm−3 (left) and ﹩{\bar{n}}_{{{\rm{H}}}_{2}}=1\times {10}^{5}﹩ cm−3 (right).

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